Mass spectrometric identification of cosmic-ray-produced neon in terrestrial rocks with multiple neon components
Mass spectrometric identification of cosmic-ray-produced neon in terrestrial rocks with multiple neon components
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DOI:
10.1016/0012-821x(93)90159-7
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发表时间:
1993-07
影响因子:
5.3
通讯作者:
S. Niedermann;T. Graf;K. Marti
中科院分区:
文献类型:
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作者:
S. Niedermann;T. Graf;K. Marti
Studies of cosmic-ray-produced nuclides in terrestrial rocks are expected to provide important geomorphological and glaciological information, such as surface exposure ages, erosion rates and extent of glacial cover. In the case of the stable nuclide21Ne, the cosmic-ray-produced component may represent but one of several components, and a component resolution based on three-isotope correlations is essential. We developed analytical techniques which permit accurate corrections for all interfering ions. We show (for our modified Nier source) that corrections for doubly charged species based on constant charge state ratios are not satisfactory. The improved techniques permit isotopic studies of < 106atoms of21Ne. The spallation ratio(22Ne/21Ne)cfrom Si was calibrated using a quartz separate from an Allan Hills sandstone and yields a value of1.243 ± 0.022. This ratio is expected to be essentially constant for terrestrial quartz samples and should be useful in component resolutions. The stepwise release of Ne at increasing temperatures shows that cosmic-ray-produced Ne is released from quartz at rather low temperatures. This permits an estimate of the activation energy for Ne diffusion in quartz (90 ± 10 kJ/mol).